C IV line profile correlations in NGC 4151

1991 ◽  
Vol 371 ◽  
pp. 136 ◽  
Author(s):  
R. P. Fahey ◽  
A. G. Michalitsianos ◽  
D. Kazanas
Keyword(s):  
1999 ◽  
Vol 523 (2) ◽  
pp. L129-L132 ◽  
Author(s):  
Jun-Xian Wang ◽  
You-Yuan Zhou ◽  
Ting-Gui Wang
Keyword(s):  

1986 ◽  
Vol 119 ◽  
pp. 351-352
Author(s):  
J. Clavel ◽  
A. Altamore ◽  
A. Boksenberg ◽  
G.E. Bromage ◽  
A. Elvius ◽  
...  

Fitting technics are applied to study the variations of the 1550 line profile and adjacent features in the IUE spectrum of the Seyfert galaxy NGC 4151, from 1978 up to 1983. New important results are found concerning the kinematics and physics of the emission line gas at a few light-days from the continuum source.


Quasars ◽  
1986 ◽  
pp. 351-352
Author(s):  
J. Clavel ◽  
A. Altamore ◽  
A. Boksenberg ◽  
G. E. Bromage ◽  
A. Elvius ◽  
...  

1987 ◽  
Vol 225 (4) ◽  
pp. 837-849 ◽  
Author(s):  
K. J. Leech ◽  
M. V. Penston ◽  
M. A. J. Snijders ◽  
T. R. Gull
Keyword(s):  

1987 ◽  
Vol 321 ◽  
pp. 251 ◽  
Author(s):  
J. Clavel ◽  
A. Altamore ◽  
A. Boksenberg ◽  
G. E. Bromage ◽  
A. Elvius ◽  
...  

1995 ◽  
Vol 453 (2) ◽  
Author(s):  
T. Yaqoob, ◽  
R. Edelson, ◽  
K. A. Weaver, ◽  
R. S. Warwick, ◽  
R. F. Mushotzky, ◽  
...  
Keyword(s):  

1994 ◽  
Vol 144 ◽  
pp. 365-367
Author(s):  
E. V. Kononovich ◽  
O. B. Smirnova ◽  
P. Heinzel ◽  
P. Kotrč

AbstractThe Hα filtergrams obtained at Tjan-Shan High Altitude Observatory near Alma-Ata (Moscow University Station) were measured in order to specify the bright rims contrast at different points along the line profile (0.0; ± 0.25; ± 0.5; ± 0.75 and ± 1.0 Å). The mean contrast value in the line center is about 25 percent. The bright rims interpretation as the bases of magnetic structures supporting the filaments is suggested.


1979 ◽  
Vol 44 ◽  
pp. 53-55
Author(s):  
R.W. Milkey ◽  
J.N. Heasley ◽  
E.J. Schmahl ◽  
O. Engvold

The effect of partial frequency redistribution in the formation of Lyman α in the chromosphere has been discussed by Milkey and Mihalas (1973) and others, and it has been shown that in this case the coherency of scattering in the wings of the line substantially influences the line profile. Although there are non-negligible sources for La photons within a prominence, a large fraction of the emergent line photons are due to scattering of photons incident on the surface of the prominence so that one expects that in a prominence the frequency redistribution processes will play an important role in determining the emergent intensity.


2006 ◽  
Vol 2006 (suppl_23_2006) ◽  
pp. 129-134 ◽  
Author(s):  
E. Schafler ◽  
K. Nyilas ◽  
S. Bernstorff ◽  
L. Zeipper ◽  
M. Zehetbauer ◽  
...  

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